Classification of BLL Blazars by Optical Activity Types

IF 0.6 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
A. M. Mickaelian, H. V. Abrahamyan, G. M. Paronyan, G. A. Mikayelyan, A. G. Sukiasyan, V. K. Mkrtchyan
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引用次数: 0

Abstract

We have carried out a spectral classification by the Activity Types for a subsample of Blazars from the BZCAT v.5 Catalogue, namely the BL Lac (BLL, Lacertids) candidates, designated in the Catalogue as BZB subtype objects. The classification is based on the Sloan Digital Sky Survey (SDSS) homogeneous medium-resolution optical spectroscopy and along with the standard BPT-type diagnostic diagrams, we have applied our newly introduced fine classification scheme with subtypes of Quasars and considering many more features. Out of 1151 BZB objects, 552 having SDSS spectra were classified. After new classification, 259 (46.1%) of 552 have not changed their optical class, and 293 (53.1%) of these objects have changed their optical class. Having this new information on the optical classification we suggest to change the classification of some objects in BZCAT: for 130 BZB objects to BZG, for 18 BZB objects to BZQ and for 145 BZB objects to BZU.

按光学活动类型对 BLL 亮星进行分类
我们对BZCAT v.5星表中的一个燃烧星子样品,即BL Lac(BLL,Lacertids)候选者,进行了活动类型的光谱分类,在星表中被指定为BZB子类型天体。我们的分类是基于斯隆数字巡天(SDSS)的同质中分辨率光学光谱,并结合标准的BPT类型诊断图,应用了我们新引入的类星体亚型精细分类方案,并考虑了更多的特征。在1151个BZB天体中,有552个具有SDSS光谱的天体被分类。经过新的分类,552个天体中有259个(46.1%)的光学分类没有改变,293个(53.1%)的光学分类发生了改变。有了这些新的光学分类信息,我们建议改变 BZCAT 中一些天体的分类:将 130 个 BZB 天体改为 BZG,将 18 个 BZB 天体改为 BZQ,将 145 个 BZB 天体改为 BZU。
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来源期刊
Astrophysics
Astrophysics 地学天文-天文与天体物理
CiteScore
0.90
自引率
20.00%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Astrophysics (Ap) is a peer-reviewed scientific journal which publishes research in theoretical and observational astrophysics. Founded by V.A.Ambartsumian in 1965 Astrophysics is one of the international astronomy journals. The journal covers space astrophysics, stellar and galactic evolution, solar physics, stellar and planetary atmospheres, interstellar matter. Additional subjects include chemical composition and internal structure of stars, quasars and pulsars, developments in modern cosmology and radiative transfer.
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